Help Shape the Future of Space Exploration

Join The Planetary Society Now  arrow.png

Join our eNewsletter for updates & action alerts

    Please leave this field empty

Headshot of Emily Lakdawalla

LPSC 2014: Water on...Vesta?

Posted by Emily Lakdawalla

21-03-2014 16:03 CDT

Topics: asteroid 4 Vesta, pretty pictures, asteroids, Dawn, explaining science, conference report

On Tuesday afternoon at the Lunar and Planetary Science Conference I spent most of my time in a session titled "Enceladus and Friends." But there was one talk that I had to go check out in another session, in which Jennifer Scully discussed possible water-carved gullies in an unusual location: within craters on Vesta. Water-carved gullies on Mars I can accept; but on an airless lumpy body? I was intrigued.

Global view of Vesta in natural color

NASA / JPL / MPS / DLR / IDA / Björn Jónsson

Global view of Vesta in natural color
Vesta is one of the more colorful asteroids in the solar system. This view is composed of 17 individual color frames, carefully assembled and draped over a digital model of the shape of Vesta. The color has been corrected to match Vesta's visible spectrum.

Scully said she had identified two distinct types of gullies on Vesta in 170 locations. Of these 170, 59 contained gullies. Most of these -- 51 of them -- were linear systems that she suggested were caused by dry flow of granular material -- basically, dust and debris flowing down slope. They are quite straight, not branching or intersecting. She found them both inside and outside craters. These sort of dry avalanches are common on airless and atmosphere-blessed bodies, large and small, across the solar system.

But in a few locations, there was a quite different type of gully: curvilinear systems of interconnected valleys, forming more complex networks. An example of this kind of gully lies within one of my favorite Vestan craters, Cornelia. The photo above has Cornelia roughly at the center. Let's zoom in:

Cornelia, a fresh crater on Vesta


Cornelia, a fresh crater on Vesta
This detail of a Dawn image shows a fresh scarp rimmed crater with a remarkable distribution of bright and dark material in its interior. Most of this bright and dark material originates from the crater rim but some originates much farther down the inwardly dipping crater walls.

And here it is again, in a high-resolution view that I put together when I played with the Dawn image data browser last fall.

Mosaic of Low-Altitude Mapping Orbit images of Cornelia crater, Vesta


Mosaic of Low-Altitude Mapping Orbit images of Cornelia crater, Vesta
This mosaic is composed of five images of Vesta captured by Dawn during its Low Altitude Mapping Orbit phase. The images were taken between January 11 and March 13, 2012. At full resolution, it is about 20 meters per pixel, covering an area about 30 kilometers across.

Scully found the curvilinear gullies in only 8 locations. All were inside young craters. Furthermore, they originated in the upper-middle walls of young craters. Where these gullies reach the floors of their craters, they end in lobate deposits, similar to Earth alluvial fans. Often, those deposits have pitted surfaces, as the floor of Cornelia does. Pitted deposits across the solar system usually indicate a place where some solid but volatile substance has turned to a gas and escaped to the vacuum. Hmmmmmmmmm......

So: What could be flowing down the crater wall, forming interconnected valleys, and creating a deposit in the floor of the crater, that then experiences some kind of degassing? One candidate is impact melt -- impacts can generate enough heat to melt the rocky surface of a planetary body. But Scully said that the morphology of both types of gullies just doesn't look like other deposits on Vesta that definitely are impact melts. Scully went through a variety of factors to see if there was anything that could explain or predict which craters would form the straight type of gullies and which would form the curvilinear type of gullies. She couldn't find anything.

So she proposed the following. Assume that there are pockets of subsurface water ice on Vesta. Other work has shown that such pockets of ice could theoretically be stable in Vesta's regolith for billions of years. The Cornelia impact would have energy to spare to melt a subsurface ice pocket.

Scully showed the locations of the eight craters with curvilinear gullies on a map. They clustered tightly in two locations. So maybe those are two locations on Vesta with deposits of subsurface ice for some reason. Because the craters in which they occur are young, there could still be water ice deposits within Vesta. Where would this ice come from? Scully pointed out that we do know that impactors have deposited carbon-rich material on Vesta; but she admitted that there was no correlation between the locations of curvilinear gullies and that material.

I found it an intriguing, though not completely convincing, talk. It's an exciting idea though -- imagine an asteroid collision, and the slow-motion excavation of a crater (slow because of the relatively low gravity), and the impact shock flashing an icy deposit into water, and it springing and tumbling down the slumping wall of the crater mixed with the cascading debris of the crater wall, the surface steaming all the way (because it's in a vacuum), all of this silent (because it's in a vacuum), the debris filling the new crater's floor, still steaming at the top while freezing toward the bottom. Periodically, rarely, a hole appears in the floor, sediment draining downward, as escaping vapor leaves a void behind.

I don't know if it's true, but it's a nice story!

See other posts from March 2014


Or read more blog entries about: asteroid 4 Vesta, pretty pictures, asteroids, Dawn, explaining science, conference report


morganism: 03/21/2014 11:59 CDT

Would like to see how those features map out against the "pressure ridges" on Vesta. It would be probable that those ridges or gouges would collapse any subsurface void features, and compress any plastic materials away from them. you could use that as a selector to look for more ?

Beemer: 03/23/2014 06:23 CDT

Yes I agree, the nature of the fall back was fluidic. As a child I had an incredible amount of fun with air and sand. I found any gas is released slowly through sand it becomes much more fluid. Certain things float and others sink. Where the "mud" rocks have cracked open on Mars but are completely obfuscated, we see no "stones"**. **An old friend and work colleague who's lifelong hobby was geology hated me using that word ;) Maybe we are seeing what was water and/or say, CO2 ice mixed in with the dust/sand? Down in Glenelg the cracks in the valley basin indeed looked like little rivulets too. Also elsewhere we see hundreds of bubble marks in the ground like remnants of small craters which I'm not so sure about. Dingo gap had an unusually hard dune like old cement. This was already dessicated. Now we are North of the Kimberly layers we see some slight movements in the dust/sand where the top is stable and the darker sand underneath has escaped. It could be from a loss of water or any frozen gaseous glue. Above all, the lower atmospheric pressure and gravity must have a huge bearing on density, pressure temperatures and friction. A hugely fascinating subject.

Bob Ware: 03/23/2014 12:47 CDT

Ceres has water source(s) that Herschel has detected. So it is possible there are pockets of ice(s) trapped and eventually released at impact (on opposite side maybe) that may trigger antipodal effects that have created what is seen.

Leave a Comment:

You must be logged in to submit a comment. Log in now.
Facebook Twitter Email RSS AddThis

Blog Search

Planetary Defense

An asteroid or comet headed for Earth is the only large-scale natural disaster we can prevent. Working together to fund our Shoemaker NEO Grants for astronomers, we can help save the world.


Featured Images

SpaceX CRS-8 landed booster
SES-10 static test fire
More Images

Featured Video

Class 9: Saturn, Uranus, and Neptune

Watch Now

Space in Images

Pretty pictures and
awe-inspiring science.

See More

Join The Planetary Society

Let’s explore the cosmos together!

Become a Member

Connect With Us

Facebook, Twitter, YouTube and more…
Continue the conversation with our online community!